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, as well as pixel size. The position of the direct beam (qz=0, q‖=0) in the pixel space of the detector need to be specified as well as the X - ray wavelength λ in units of Å. The aforementioned distortion ...
necessary to produce the observed H2 and [Fe ii] line emission. galaxies: active, galaxies: individual (NGC 1275), galaxies: kinematics and dynamics 1 INTRODUCTION Perseus is the X - ray brightest known galaxy ...
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